🔗 Tsiolkovsky Rocket Equation

🔗 Spaceflight 🔗 Physics 🔗 Rocketry

The Tsiolkovsky rocket equation, classical rocket equation, or ideal rocket equation is a mathematical equation that describes the motion of vehicles that follow the basic principle of a rocket: a device that can apply acceleration to itself using thrust by expelling part of its mass with high velocity can thereby move due to the conservation of momentum.

Δ v = v e ln m 0 m f = I sp g 0 ln m 0 m f {\displaystyle \Delta v=v_{\text{e}}\ln {\frac {m_{0}}{m_{f}}}=I_{\text{sp}}g_{0}\ln {\frac {m_{0}}{m_{f}}}}

where:

Δ v   {\displaystyle \Delta v\ } is delta-v – the maximum change of velocity of the vehicle (with no external forces acting).
m 0 {\displaystyle m_{0}} is the initial total mass, including propellant, also known as wet mass.
m f {\displaystyle m_{f}} is the final total mass without propellant, also known as dry mass.
v e = I sp g 0 {\displaystyle v_{\text{e}}=I_{\text{sp}}g_{0}} is the effective exhaust velocity, where:
I sp {\displaystyle I_{\text{sp}}} is the specific impulse in dimension of time.
g 0 {\displaystyle g_{0}} is standard gravity.
ln {\displaystyle \ln } is the natural logarithm function.

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